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How Solar Storms Affect Your Phone

Interactive passage with audio narration, comprehension questions, and printable PDF.

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Grades 5–8ScienceElaEnglish · SpanishInteractive · Printable
Aligned toMS-ESS1-3
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About this printable How Solar Storms Affect Your Phone science reading passage, NGSS-aligned (Grades 5-8)

This 400-500 word informational science reading passage explains how solar storms affect everyday technology like phones and GPS systems. Aligned to NGSS MS-ESS1-3 and DCI MS-ESS1.B, the passage connects space weather to real-life experiences students can relate to. The content begins with familiar scenarios like GPS glitches and flight reroutes, then explains the scientific process: the Sun releases bursts of charged particles that reach Earth and disrupt the magnetic field, affecting satellites, power grids, and radio signals. Students learn about coronal mass ejections, the magnetosphere, and how scientists monitor space weather. The passage includes audio integration for accessibility, a simplified version for struggling readers, Spanish translations, a comprehensive glossary, multiple-choice questions, writing activities, and graphic organizers. This standards-aligned resource helps middle school students understand how events in space directly impact technology in their daily lives.
Written by Workybooks TeamPublished by Workybooks
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Sample passage and quiz from How Solar Storms Affect Your Phone

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How Solar Storms Affect Your Phone

Close-up of hands using a map app on a smartphone outdoors, showcasing GPS navigation.

Evidence shows that solar storms can interfere with satellites orbiting Earth. GPS satellites may send inaccurate signals, causing navigation systems to malfunction.  Image by Ingo Joseph / Pexels.

Have you ever noticed your GPS suddenly showing the wrong location? Perhaps a flight was rerouted unexpectedly, or you saw news about the northern lights appearing in unusual places. These events may seem unrelated, but they share a common cause: solar storms. The Sun occasionally releases powerful bursts of charged particles into space. When these particles reach Earth, they can disrupt the technology we rely on every day.

Solar storms begin with activity on the Sun's surface. Scientists observe that the Sun releases massive clouds of charged particles called coronal mass ejections. These ejections travel through space at speeds up to several million miles per hour. When they reach Earth, usually within one to three days, they interact with our planet's magnetic field. This interaction can compress and distort the magnetic field, creating what scientists call space weather. The magnetosphere, which normally protects Earth from harmful radiation, becomes disturbed during these events.

The effects of solar storms reach far beyond pretty light displays in the sky. Evidence shows that these storms can interfere with satellites orbiting Earth. GPS satellites may send inaccurate signals, causing navigation systems to malfunction. Radio communications can fade or become filled with static. Power grids on Earth's surface may experience surges that can damage transformers. In March 1989, a powerful solar storm caused a blackout in Quebec, Canada, leaving six million people without electricity for nine hours. Airlines sometimes reroute flights over polar regions to avoid communication problems and increased radiation exposure during major solar storms.

Understanding solar storms matters because our society depends heavily on technology vulnerable to space weather. Scientists monitor the Sun constantly using spacecraft and ground-based instruments. When they detect a coronal mass ejection heading toward Earth, they can issue warnings. These warnings give satellite operators time to protect their equipment and power companies time to prepare their systems. As we use more satellites for communication, navigation, and weather forecasting, predicting space weather becomes increasingly important for protecting the technology in our pockets and homes.

Interesting Fact: The largest recorded solar storm, called the Carrington Event, occurred in 1859. Telegraph systems worldwide sparked and caught fire, and auroras were visible as far south as the Caribbean.

Comprehension quiz (10 questions)

1. What are coronal mass ejections?

Massive clouds of charged particles released by the Sun
Satellites that monitor space weather
Power surges in electrical grids
Northern lights visible from Earth

2. How long does it typically take for charged particles from the Sun to reach Earth?

A few minutes
One to three days
Several weeks
About one month

3. What happened in Quebec, Canada in March 1989?

A tornado destroyed power lines
A solar storm caused a nine-hour blackout
The northern lights were seen for the first time
All satellites stopped working permanently

4. In the passage, what does the word 'magnetosphere' refer to?

The part of Earth's magnetic field that protects the planet
A type of solar storm
A device used to measure radiation
The surface of the Sun

5. What does 'space weather' mean in this passage?

Temperature changes in outer space
Conditions in space caused by solar activity that affect Earth
Weather patterns on other planets
The movement of satellites around Earth

6. Based on the passage, why do airlines sometimes reroute flights during solar storms?

To save fuel
To see the northern lights
To avoid communication problems and radiation exposure
To fly faster

7. Which statement best explains why scientists monitor the Sun constantly?

To study the temperature of space
To predict when the Sun will explode
To warn about incoming solar storms so technology can be protected
To count the number of stars in the galaxy

8. How can solar storms affect GPS satellites?

They cause satellites to fall out of orbit
They make satellites send inaccurate signals
They improve GPS accuracy
They have no effect on satellites

9. True or False: The Carrington Event in 1859 was the largest recorded solar storm.

True
False

10. True or False: Solar storms only create northern lights and have no other effects on Earth.

True
False
Who it's for

Perfect for the way you teach

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